ε Trianguli Australis (epsilon Trianguli Australis)

ε Trianguli Australis is a double giant star of spectral class K1 in the constellation of Triangulum Australe.

ε Trianguli Australis visual magnitude is 4.11. Because of its moderate brightness, ε Trianguli Australis is easily visible to the naked eye from locations with dark skies, while it might be barely visible, or not visible at all, from light-polluted skies.

Celestial Coordinates

Apparent

J2000

Galactic Coordinates

Finder Chart

Magnitude, Color, Spectral Class

The red dot in the diagram below shows where ε Trianguli Australis is situated in the Hertzsprung–Russell diagram.

Star System Properties

ε Trianguli Australis is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the ε Trianguli Australis double sysyem:

Distance, Radial Speed, Proper Motion

ε Trianguli Australis is distant 216.04 light years from the Sun and it is moving towards the Sun at the speed of 16 kilometers per second.

Alternative Designations

Visibility from Your Location

ε Trianguli Australis (epsilon Trianguli Australis) is currently not visible from Ludgeřovice, Repubblica Ceca